Axiorecombination: A new mechanism for stellar axion production

Details Axiorecombination: A new mechanism for stellar axion production Axiorecombination: A new mechanism for stellar axion production

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phlb..179..223d&link_type=abstract

Physics Letters B, Volume 179, Issue 3, p. 223-227.

Physics

13

Scientific paper

Axiorecombination, e- + Z --> (e-, Z) + a, is considered as a source of light pseudoscalar axions in stars. This process dominates the energy loss in axions for low-mass main-sequence stars, M <~ 0.2M⊚. For the sun, axiorecombination accounts for ~1/4 of total axion flux at energies above ~2 keV.
National Science and Engineering Research Council (Canada) Postgraduate Scholar.

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